Publications
Detailed Information
The Velocity Dispersion Function for Quiescent Galaxies in Nine Strong-lensing Clusters
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Sohn, Jubee | - |
dc.contributor.author | Fabricant, Daniel G. | - |
dc.contributor.author | Geller, Margaret J. | - |
dc.contributor.author | Hwang, Ho Seong | - |
dc.contributor.author | Diaferio, Antonaldo | - |
dc.date.accessioned | 2024-05-03T02:26:34Z | - |
dc.date.available | 2024-05-03T02:26:34Z | - |
dc.date.created | 2024-05-03 | - |
dc.date.created | 2024-05-03 | - |
dc.date.issued | 2020-10 | - |
dc.identifier.citation | ASTROPHYSICAL JOURNAL, Vol.902 No.1 | - |
dc.identifier.issn | 0004-637X | - |
dc.identifier.uri | https://hdl.handle.net/10371/200743 | - |
dc.description.abstract | We measure the central stellar velocity dispersion function for quiescent galaxies in a set of nine northern clusters in the redshift range 0.18 < z < 0.29 and with strong lensing arcs in Hubble Space Telescope images. The velocity dispersion function links galaxies directly to their dark matter halos. From dense SDSS and MMT/Hectospec spectroscopy, we identify 222-463 spectroscopic members in each cluster. We derive physical properties of cluster members including redshift, D(n)4000, and central stellar velocity dispersion and we include a table of these measurements for 3419 cluster members. We construct the velocity dispersion functions for quiescent galaxies with D(n)4000 > 1.5 and within R-200. The cluster velocity dispersion functions all show excesses at sigma greater than or similar to 250 kms(-1) compared to the field velocity dispersion function. The velocity dispersion function slope at large velocity dispersion (sigma > 160 km s(-1)) is steeper for more massive clusters, consistent with the trend observed for cluster luminosity functions. The spatial distribution of galaxies with large velocity dispersion at radii larger than R-200 further underscores the probable major role of dry mergers in the growth of massive cluster galaxies during cluster assembly. | - |
dc.language | 영어 | - |
dc.publisher | IOP PUBLISHING LTD | - |
dc.title | The Velocity Dispersion Function for Quiescent Galaxies in Nine Strong-lensing Clusters | - |
dc.type | Article | - |
dc.identifier.doi | 10.3847/1538-4357/abb23b | - |
dc.citation.journaltitle | ASTROPHYSICAL JOURNAL | - |
dc.identifier.wosid | 000576334400001 | - |
dc.identifier.scopusid | 2-s2.0-85092645950 | - |
dc.citation.number | 1 | - |
dc.citation.volume | 902 | - |
dc.description.isOpenAccess | Y | - |
dc.contributor.affiliatedAuthor | Sohn, Jubee | - |
dc.type.docType | Article | - |
dc.description.journalClass | 1 | - |
dc.subject.keywordPlus | DARK-MATTER HALOES | - |
dc.subject.keywordPlus | STELLAR MASS | - |
dc.subject.keywordPlus | FUNDAMENTAL PLANE | - |
dc.subject.keywordPlus | ENVIRONMENTAL DEPENDENCE | - |
dc.subject.keywordPlus | COSMOLOGICAL SIMULATIONS | - |
dc.subject.keywordPlus | PHYSICAL PROCESSES | - |
dc.subject.keywordPlus | ELLIPTIC GALAXIES | - |
dc.subject.keywordPlus | INFALL REGIONS | - |
dc.subject.keywordPlus | STAR-FORMATION | - |
dc.subject.keywordPlus | DIFFUSE LIGHT | - |
dc.subject.keywordAuthor | Early-type galaxies | - |
dc.subject.keywordAuthor | Galaxy clusters | - |
dc.subject.keywordAuthor | Luminosity function | - |
dc.subject.keywordAuthor | Galaxy mass distribution | - |
dc.subject.keywordAuthor | Redshift surveys | - |
- Appears in Collections:
- Files in This Item:
- There are no files associated with this item.
Item View & Download Count
Items in S-Space are protected by copyright, with all rights reserved, unless otherwise indicated.